We provide the first solar system wide compendium of speleogenic processes and products.
An examination of 15 solar system bodies revealed that six cave‐forming processes occur …

Titan was a mostly unknown world prior to the Cassini spacecraft's arrival in July 2004. We
review the major scientific advances made by Cassini's Titan Radar Mapper (RADAR) …

Titan has an active methane-based hydrologic cycle that has shaped a complex geologic
landscape, making its surface one of most geologically diverse in the Solar System. Despite …

Abstract Thanks to the Cassini–Huygens mission, Titan, the pale orange dot of Pioneer and
Voyager encounters, has been revealed to be a dynamic, hydrologically shaped, organic …

Triboelectric, or frictional, charging is a ubiquitous yet poorly understood phenomenon in
granular flows. Recognized in terrestrial volcanic plumes and sand storms, such …

Titan is a sedimentary world, with lakes, rivers, canyons, fans, dissected plateaux, and sand
dunes. Sediments on Saturn's moon are thought to largely consist of mechanically weak …

Titan is a hydrologically active world, with dozens of alluvial fans that are evidence of
sediment transport from high to low elevations. However, the distribution and requirements …

We present a geomorphologic map of Titan's polar terrains. The map was generated from a
combination of Cassini Synthetic Aperture Radar (SAR) and Imaging Science Subsystem …

Titan is unique in the solar system: it is an ocean world, an icy world, an organic world, and
has a dense atmosphere. It is a geologically active world as well, with ongoing exogenic …

We propose that cycling hydrocarbon rains on Saturn's moon Titan are likely to create
subsurface conduits through dissolution geology of the extensive organic and largely …